On the Early Thermal Processing of Planetesimals during and after the Giant Planet Instability

Born as ice-rich planetesimals, cometary nuclei were gravitationally scattered onto their current orbits in the Kuiper Belt and the Oort Cloud during the giant planets’ dynamical instability in the early stages of our solar system’s history. Here, we model the thermal evolution of planetesimals duri...

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書誌詳細

主要な著者:	Anastasios Gkotsinas, David Nesvorný, Aurélie Guilbert-Lepoutre, Sean N. Raymond, Nathan Kaib
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2024-01-01
シリーズ:	The Planetary Science Journal
主題:	Long period comets Short period comets Planetesimals Comet dynamics Comet nuclei Comet volatiles
オンライン･アクセス:	https://doi.org/10.3847/PSJ/ad7f4e
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